English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

We present a transmission spectrum for the Neptune-size exoplanet HD 106315 cfrom optical to infrared wavelengths based on transit observations from theHubble Space Telescope/Wide Field Camera 3, K2, and Spitzer. The spectrum showstentative evidence for a water absorption feature in the $1.1 - 1.7\mu$mwavelength range with a small amplitude of 30 ppm (corresponding to just $0.8\pm 0.04$ atmospheric scale heights). Based on an atmospheric retrievalanalysis, the presence of water vapor is tentatively favored with a Bayesfactor of 1.7 - 2.6 (depending on prior assumptions). The spectrum is mostconsistent with either enhanced metallicity, high altitude condensates, orboth. Cloud-free solar composition atmospheres are ruled out at $>5\sigma$confidence. We compare the spectrum to grids of cloudy and hazy forward modelsand find that the spectrum is fit well by models with moderate cloud lofting orhaze formation efficiency, over a wide range of metallicities ($1 - 100\times$solar). We combine the constraints on the envelope composition with an interiorstructure model and estimate that the core mass fraction is $\gtrsim0.3$. Witha bulk composition reminiscent of that of Neptune and an orbital distance of0.15 AU, HD 106315 c hints that planets may form out of broadly similarmaterial and arrive at vastly different orbits later in their evolution.

Tentative Evidence for Water Vapor in the Atmosphere of the Neptune-Size Exoplanet HD 106315 c